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相关论文: Gauss-Bonnet Boson Stars with a Single Killing Vec…

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We numerically construct asymptotically anti-de Sitter boson star solutions using a minimally coupled $\frac{D-1}{2}$-tuplet complex scalar field in $D=5,7,9,11$ dimensions. The metric admits multiple Killing vector fields in general,…

高能物理 - 理论 · 物理学 2014-02-19 Sean Stotyn , C. Danielle Leonard , Marius Oltean , Laura J. Henderson , Robert B. Mann

We complete the analysis of part I in this series (Ref. \cite{Stotyn:2013yka}) by numerically constructing boson stars in 2+1 dimensional Einstein gravity with negative cosmological constant, minimally coupled to a complex scalar field.…

高能物理 - 理论 · 物理学 2014-02-19 Sean Stotyn , Melanie Chanona , Robert B. Mann

We construct boson stars in (4+1)-dimensional Gauss-Bonnet gravity. We study the properties of the solutions in dependence on the coupling constants and investigate these in detail. While the "thick wall" limit is independent of the value…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Betti Hartmann , Juergen Riedel , Raluca Suciu

In this paper, we have constructed Boson star (BS) solutions in four dimensional scalar-Gauss-Bonnet (sGB) theory. In order to have non-trivial effect from Gauss-Bonnet term, we invoked non-minimal coupling between a complex scalar field…

广义相对论与量子宇宙学 · 物理学 2017-01-25 Vishal Baibhav , Debaprasad Maity

We construct rotating boson stars in (4+1)-dimensional asymptotically Anti-de Sitter space-time (aAdS) with two equal angular momenta that are composed out of a massive and self-interacting scalar field. These solutions possess a single…

广义相对论与量子宇宙学 · 物理学 2015-09-02 Yves Brihaye , Betti Hartmann , Jürgen Riedel

In recent years, there has been a growing interest in stellar modelling in the framework of Einstein-Gauss-Bonnet gravity. In this paper, for a relativistic star in static equilibrium, we invoke the $5$ dimensional Einstein-Gauss-Bonnet…

广义相对论与量子宇宙学 · 物理学 2023-06-22 Soumik Bhattacharya , Suntharalingam Thirukkanesh , Ranjan Sharma

A self-interacting SU(2)-doublet of complex scalar fields, minimally coupled to Einstein-Gauss-Bonnet gravity is considered in five space-time dimensions. The classical equations admit two families of solitons corresponding to spinning and…

广义相对论与量子宇宙学 · 物理学 2014-06-11 Yves Brihaye , Jürgen Riedel

We study axially symmetric solutions of the Einstein-Maxwell-Klein-Gordon equations describing spinning gauged boson stars in a 3+1 dimensional asymptotically AdS spacetime. These smooth horizonless solutions possess an electric charge and…

广义相对论与量子宇宙学 · 物理学 2015-06-17 Olga Kichakova , Jutta Kunz , Eugen Radu

We construct supersymmetric Q-balls and boson stars in (d+1) dimensions. These non-topological solitons are solutions of a scalar field model with global U(1) symmetry and a scalar field potential that appears in gauge-mediated…

高能物理 - 理论 · 物理学 2013-05-30 Betti Hartmann , Juergen Riedel

We consider a model with two real Maxwell fields (or equivalently, a complex Maxwell field) minimally coupled to Einsteins gravity with a negative cosmological constant in four spacetime dimensions. Assuming a specific harmonic dependence…

广义相对论与量子宇宙学 · 物理学 2024-05-20 Carlos Herdeiro , Hyat Huang , Jutta Kunz , Eugen Radu

We consider boson star solutions in a $D$-dimensional, asymptotically anti-de Sitter spacetime and investigate the influence of the cosmological term on their properties. We find that for $D>4$ the boson star properties are close to those…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Dumitru Astefanesei , Eugen Radu

In the frame of Gauss-Bonnet gravity and in the limit of $D\to 4$, based on the fact that spherically symmetric solution derived using any of regularization schemes will be the same form as the original theory…

广义相对论与量子宇宙学 · 物理学 2022-03-07 G. G. L. Nashed , S. D. Odintsov , V. K. Oikonomou

We extend the recent D=5 results of Dias, Horowitz and Santos by finding asymptotically AdS rotating black hole and boson star solutions with scalar hair in arbitrary odd spacetime dimension. Both the black holes and the boson stars are…

高能物理 - 理论 · 物理学 2012-02-16 Sean Stotyn , Miok Park , Paul L. McGrath , Robert B. Mann

We review particle-like configurations of complex scalar field, localized by gravity, so-called boson stars. In the simplest case, these solutions posses spherical symmetry, they may arise in the massive Einstein-Klein-Gordon theory with…

广义相对论与量子宇宙学 · 物理学 2022-04-14 Yakov Shnir

We consider compact boson stars that arise for a V-shaped scalar field potential. They represent a one parameter family of solutions of the scaled Einstein-signum-Gordon equations. We analyze the physical properties of these solutions and…

广义相对论与量子宇宙学 · 物理学 2015-06-05 Betti Hartmann , Burkhard Kleihaus , Jutta Kunz , Isabell Schaffer

Different types of gravitating compact objects occuring in d=5 space-time are considered: boson stars, hairy black holes and perfect fluid solutions. All these solutions of the Einstein equations coupled to matter have well established…

广义相对论与量子宇宙学 · 物理学 2016-07-27 Y. Brihaye , T. Delsate

We study axially symmetric multi-soliton solutions of a complex scalar field theory with a sextic potential, minimally coupled to Einstein's gravity. These solutions carry no angular momentum and can be classified by the number of nodes of…

广义相对论与量子宇宙学 · 物理学 2021-03-31 C. A. R. Herdeiro , J. Kunz , I. Perapechka , E. Radu , Y. Shnir

The study of the properties and dynamics of self-gravitating bosonic objects in Einstein gravity was conducted. We studied self-coupled boson stars and determined the quasinormal mode (QNM) frequencies of stable boson stars in spherical…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Jayashree Balakrishna

We show that complex, massive spin-1 fields minimally coupled to Einstein's gravity with a negative cosmological constant, admit asymptotically anti-de Sitter self-gravitating solutions. Focusing on 4-dimensional spacetimes, we start by…

广义相对论与量子宇宙学 · 物理学 2016-09-26 Miguel Duarte , Richard Brito

We study boson shells and boson stars in a theory of complex scalar field coupled to the $U(1)$ gauge field $A_{\mu}$ and Einstein gravity with the potential: $V(|\Phi|) := \frac{1}{2} m^{2} \left(|\Phi|+ a \right)^2$. This could be…

高能物理 - 理论 · 物理学 2016-06-08 Sanjeev Kumar , Usha Kulshreshtha , Daya Shankar Kulshreshtha
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